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SEARCH FOR EXTRATERRESTRIAL ANTINEUTRINO SOURCES WITH THE KamLAND DETECTOR
Journal article   Open access   Peer reviewed

SEARCH FOR EXTRATERRESTRIAL ANTINEUTRINO SOURCES WITH THE KamLAND DETECTOR

A. Gando, Y. Gando, K. Ichimura, H. Ikeda, K. Inoue, Y. Kibe, Y. Kishimoto, M. Koga, Y. Minekawa, T. Mitsui, …
The Astrophysical journal, v 745(2)
01 Feb 2012
url
https://doi.org/10.1088/0004-637x/745/2/193View
Published, Version of Record (VoR)Open Access (License Unspecified) Open
url
https://doi.org/10.1088/0004-637X/745/2/193View
Published, Version of Record (VoR) Open

Abstract

Astronomy & Astrophysics Physical Sciences Science & Technology
We present the results of a search for extraterrestrial electron antineutrinos ((nu) over bar (e)'s) in the energy range 8.3 MeV E-<(nu) over bare < 31.8 MeV using the KamLAND detector. In an exposure of 4.53 kton-year, we identify 25 candidate events. All of the candidate events can be attributed to background, most importantly neutral current atmospheric neutrino interactions, setting an upper limit on the probability of B-8 solar nu(e)'s converting into nu(e)'s at 5.3 x 10(-5) (90% CL), if we assume an undistorted nu(e) shape. This limit corresponds to a solar nu(e) flux of 93 cm(-2) s(-1) or an event rate of 1.6 events (kton-year)(-1) above the energy threshold (E-<(nu)over bar>e >= 8.3 MeV). The present data also allows us to set more stringent limits on the diffuse supernova neutrino flux and on the annihilation rates for light dark matter particles.

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